Recent Events Reported by Observers
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Detected by Jean-Pierre Wuelser, Submitted at 2017-11-15T22:18:10
2017-11-13T05:16:26 --> 2017-11-13T05:51:14
Last of three small eruptions observed within a 4-hour period. The SG slit covered each at a different stage of the eruption.
Detected by Jean-Pierre Wuelser, Submitted at 2017-11-15T22:11:29
2017-11-13T03:57:59 --> 2017-11-13T04:23:09
Second of three small eruptions observed within a 4-hour period. The SG slit covered each at a different stage of the eruption.
Detected by Jean-Pierre Wuelser, Submitted at 2017-11-15T22:07:52
2017-11-13T02:12:31 --> 2017-11-13T02:37:41
First of three small eruptions observed within a 4-hour period. The SG slit covered each at a different stage of the eruption.
Detected by gchintzo, Submitted at 2017-11-07T22:23:06
2017-11-05T00:00:09 --> 2017-11-07T00:00:09
This is the long and narrow coronal hole seen over the previous days. As the sun rotates this coronal hole seems to be an extension of the north polar coronal hole.
Detected by gchintzo, Submitted at 2017-11-07T22:07:12
2017-11-02T14:30:09 --> 2017-11-03T20:20:09
A coronal hole (dark region on the North East quadrant of the solar disk) is accompanied by two filaments running parallel to it at higher latitudes. As the time goes by, the high-latitude filament erupts folllowed by the one nearest to the coronal hole ~10 hours later. No CME was identified with SOHO/LASCO; therefore, the eruptions were not ejective but rather contained in the low solar corona.
Detected by gchintzo, Submitted at 2017-11-07T21:46:05
2017-11-02T14:30:09 --> 2017-11-03T20:20:09
The source region for a CME eruption seen from SOHO/LASCO (http://spaceweather.gmu.edu/seeds/dailymkmovie.php?cme=20171103&r) at the West limb of the sun.
Detected by Donald Schmit, Submitted at 2017-11-06T20:24:23
2017-11-05T20:28:29 --> 2017-11-05T20:54:48
This burst seems to have a dark loop connected to it in the Mg II heliogram.
Detected by Donald Schmit, Submitted at 2017-11-06T20:15:34
2017-11-05T05:43:42 --> 2017-11-05T06:01:49
Unwinding maybe. Seen in both Si IV and Mg II SJ. Full readout.
Detected by Donald Schmit, Submitted at 2017-11-06T14:41:33
2017-11-02T19:05:19 --> 2017-11-02T19:51:49
This filament is strongest in Mg II SJI, Si IV you see mostly loops. Multiple eclipse separated OBS exist
Detected by Donald Schmit, Submitted at 2017-11-06T14:15:19
2017-11-01T08:00:49 --> 2017-11-01T08:16:43
Twisting. During SAA. Raster ends early
Detected by Donald Schmit, Submitted at 2017-11-06T14:04:12
2017-10-31T22:00:49 --> 2017-10-31T22:21:00
Interesting Mg II heliogram structure. Decaying AR. Single raster
Detected by gchintzo, Submitted at 2017-11-03T00:48:13
2017-10-31T16:20:09 --> 2017-11-01T03:40:09
Recurring/homologous jet activity in the south pole of the sun. Occasionally, absorbing material (mini-filament) is seen to lift in tandem to the jet activity.
Detected by gchintzo, Submitted at 2017-11-03T00:31:54
2017-10-30T11:30:09 --> 2017-11-01T08:40:09
A quiescent filament viewed at the solar limb (dark "tornado"-like features presumably are cool material sitting at one section of the structure). The filament and its remote connectivities is seen to progressively lift until a certain height where it accelerates as an eruption. This event is associated with a narrow-angle, jet-like CME seen by SOHO/LASCO (see http://spaceweather.gmu.edu/seeds/dailymkmovie.php?cme=20171101&r).
Detected by gchintzo, Submitted at 2017-11-03T00:21:33
2017-10-30T00:00:09 --> 2017-10-31T02:30:09
A narrow but elongated coronal hole in the south hemisphere of the sun. Note the presence of a flipped J-shaped filament very close to the coronal hole's west boundary.
Detected by Jakub Prchlik, Submitted at 2017-10-25T18:19:14
2017-10-20T13:20:38 --> 2017-10-20T14:30:06
During a coordinated filament barb observation with Hinode (SOT, XRT, and EIS), IRIS observed a material flow coincident with a filament activation visible in X-rays. Only 1330 captures the flow in IRIS.
Detected by Jakub Prchlik, Submitted at 2017-10-25T17:56:46
2017-10-19T23:50:18 --> 2017-10-20T00:08:46
All SJIs show a jet just over the west limb and north of AR 12684. The slit captures some of the spire, which causes broad emission in a number of spectral lines off the limb.
Detected by Jakub Prchlik, Submitted at 2017-10-25T17:48:15
2017-10-19T02:19:12 --> 2017-10-19T02:36:09
Brightening occurs on North Pole QS/CH boundary. The brightening creates broad spectral lines of C II (1336) and Si IV (1394).
Detected by Jakub Prchlik, Submitted at 2017-10-25T17:34:14
2017-10-17T11:14:51 --> 2017-10-17T11:28:58
A brightening in a coronal plume produces broad spectral lines in C II (1336) and Si IV (1405). The brightening occurred during a coordinated observation with Hinode SOT.
Detected by Lakshmi Pradeep Chitta, Submitted at 2017-10-25T08:41:53
2017-10-14T05:06:43 --> 2017-10-14T06:25:53
The slit caught the axis of this ephemeral region. The transition region at the Northern region of this bipole shows a variety of broad line profiles similar to those seen in explosive events and ultraviolet bursts.
Detected by Lakshmi Pradeep Chitta, Submitted at 2017-10-25T08:22:05
2017-10-14T01:04:06 --> 2017-10-14T03:25:48
The slit caught a variety of turbulent plasma motions in this filament. The slit-jaw movies show a wider view of the filament and its evolution.
